"Non-1/r" Newtonian gravitation and stellar structure
Seidov, Zakir F.
Original · EN
Some analytical spherical-symmetric equilibrium solutions are cosidered in the Newtonian theory of gravitation with deviations from 1/r law. Stability of star against a first-order phase-transition is shown to be particularly influenced by the deviations of degree in the power-law potential.
English translation
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